Ultra high energy neutrinos from supernova remnants

Published under licence by IOP Publishing Ltd
, , Citation Mou Roy 1999 J. Phys. G: Nucl. Part. Phys. 25 129 DOI 10.1088/0954-3899/25/1/011

Download Article PDF

Article metrics

91 Total downloads

Share this article

Author affiliations

1 MS 50-245, Lawrence Berkeley National Laboratory, One Cyclotron Road, Berkeley, CA 94720, USA

Dates

  1. Received 15 June 1998

Buy this article in print

Journal RSS
Sign up for new issue notifications
0954-3899/25/1/129

Abstract

In this paper we discuss possible ultra high energy ( TeV) neutrino emission from supernova remnants (SNRs), specifically the hadronic gamma-ray production models. Recent very high energy (VHE) gamma-ray observation from SNRs is the main motivation behind this study.

Export citation and abstract BibTeX RIS

Previous article in issue
Next article in issue
Please wait… references are loading.
10.1088/0954-3899/25/1/011